Relativistic collapse of stellar clusters after loss of stability

Details Relativistic collapse of stellar clusters after loss of stability Relativistic collapse of stellar clusters after loss of stability

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.147..121b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 147, no. 1, Aug. 1988, p. 121-135.

Astronomy and Astrophysics

Astrophysics

3

Astrodynamics, Gravitational Collapse, Relativistic Effects, Star Clusters, Dynamic Stability, Flow Charts, Integral Equations, Maxwell-Boltzmann Density Function, Stellar Motions

Scientific paper

An integral calculation technique is used to explore the dynamics of spherically-symmetrical relativistic stellar clusters with initially truncated Maxwellian distributions and initially self-similar distributions of stars. It is demonstrated that the main part of the clusters collapses rapidly. In the ensuing period, which is several times greater than the first stage, the main part of the remaining mass collapses and the quickest particles escape the system.

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